activity
20002009
most citedThree-Dimensional MHD Simulation of the 2003 October 28 Coronal Mass Ejection: Comparison with LASCO Coronagraph Observations

169 citations · 315 across the 4 of their papers we have counts for

collaborators

7 papers

astro-ph.EP2009118 cited

A model of acceleration of Anomalous Cosmic Rays by Reconnection in the Heliosheath

A. Lazarian, M. Opher

We discuss a model of cosmic ray acceleration that accounts for the observations of anomalous cosmic rays by Voyager 1 and 2. The model appeals to fast magnetic reconnection rather…

astro-ph200825 cited

Properties and selected implications of magnetic turbulence for interstellar medium, Local Bubble and solar wind

A. Lazarian, A. Beresnyak, H. Yan +2

Astrophysical fluids, including interstellar and interplanetary medium, are magnetized and turbulent. Their appearance, evolution, and overall properties are determined by the magn…

astro-ph2008169 cited

Three-Dimensional MHD Simulation of the 2003 October 28 Coronal Mass Ejection: Comparison with LASCO Coronagraph Observations

Ward Manchester, Angelos Vourlidas, Gabor Toth +6

We numerically model the coronal mass ejection (CME) event of October 28, 2003 that erupted from active region 10486 and propagated to Earth in less than 20 hours causing severe ge…

astro-ph20063 cited

Global Asymmetry of the Heliosphere

Merav Opher, Edward C. Stone, Paulett C. Liewer +1

Opher et al. 2006 showed that an interstellar magnetic field parallel to the plane defined by the deflection of interstellar hydrogen atoms can produce a north/south asymmetry in t…

astro-ph2004

Magnetic Effects Change Our View of the Heliosheath

M. Opher, P. C. Liewer, M. Velli +5

There is currently a controversy as to whether Voyager 1 has already crossed the Termination Shock, the first boundary of the Heliosphere. The region between the Termination Shock…

astro-ph2004

Magnetic Effects at the Edge of the Solar System: MHD Instabilities, the de Laval nozzle Effect and an Extended Jet

M. Opher, P. C. Liewer, M. Velli +6

To model the interaction between the solar wind and the interstellar wind, magnetic fields must be included. Recently Opher et al. 2003 found that, by including the solar magnetic…